Special interest has been recently devoted to the quaternary material Ag2ZnSnS4 (AZTS) due to its remarkable electrical and optical properties. Our study proposes a new method for the synthesis of Ag2ZnSnS4 thin films by thermal vacuum evaporation on soda-lime glass (SLG) substrates by tuning their thickness. Structural characterization of thin films, performed by X-ray diffraction and Raman spectroscopy, confirmed the presence of the AZTS stannite phase with the appearance of the Ag8SnS6 secondary phase. As the thickness increases, a transition from amorphous to polycrystalline state appears in the XRD spectra, along with an increase in intensity related to a refinement of the preferential peak (112), an increase in crystallite size and a decrease in stress and dislocations. Compositional analysis confirms the stoichiometric composition of the films. Atomic Force Microscopy (AFM) and Scanning Electron Microscopy (SEM) reveal a strong thickness dependence of the film on the surface structure. Moreover, the thickness affects significantly the optical properties of films. In particular, an increase of the absorption coefficients associated with a decrease of the direct gap energy and the Urbach energy is observed with increasing thickness. The optical and dielectric constants have been studied and discussed in more detail based on the single oscillator model proposed by Wemple DiDomenico and other models. The static refractive indices as well as the static dielectric constant of the layers show a slight increase with layer thickness, in contrast to the oscillator energy. Finally, all samples display n-type conductivity according to the hot probe experiment. Such attractive characteristics can be useful to further improve the efficiency of thin film solar cells by adjusting the thin film thickness.
Read full abstract